Why Does the Time/Energy Uncertainty Principle Suggest a Lower Bound in Δt?

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I don't know much about brackets and Hamiltonians, but there is a much simpler aspect of the time / energy uncertainty discussion that confuses me. It has to do with the sign of the uncertainty. [Disclaimer: Purists, please bear with me for a moment as I hash out my point heuristically.]

Here's the typical argument that I hear against the vacuum fluctuation hypothesis of the Big Bang: The energy of a system can be "unknown / inconstant / immeasurable / whatever" within a range of values ΔE, but ONLY FOR LESS TIME than Δt. Larger energy fluctuations are doomed to a shorter lifespan. So a fluctuation the size of the universe would have a Δt of about one googolth of a second. (Perhaps the only opportunity I'll ever have to use the fraction "one googolth"!)

But the damn formula has a GREATER THAN sign in it! On its face mathematically, the inequality shows us that Δt must be LONGER than h/ΔE. Why do discussions of the principle always invoke an upper bound, when the formula gives a lower bound? Is there indeed an upper bound on ΔEΔt? Or is this inequality understood to mean "greater than but approximately equal to?"
 
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Most importantly, what does this mean for the hypothesis of a vacuum fluctuation as the origin of the universe? Is it ruled out by the time/energy uncertainty principle?
 
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If we release an electron around a positively charged sphere, the initial state of electron is a linear combination of Hydrogen-like states. According to quantum mechanics, evolution of time would not change this initial state because the potential is time independent. However, classically we expect the electron to collide with the sphere. So, it seems that the quantum and classics predict different behaviours!
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